Solar System: Things To Know This Week

Tracking a Warming Arctic – From Underground to High in the Sky

The Arctic is warming much faster than the rest of Earth. This warming is creating big and small changes, some of which could ripple beyond the planet’s frozen regions and affect us world-wide – possibly raising sea levels, increasing greenhouse warming and affecting wildlife.

Our Arctic Boreal Vulnerability Experiment, known as ABoVE, just began a 10-year mission in Alaska and western Canada, studying these changes.

Underground: Permafrost is the layer of frozen soil beneath some Arctic forests and tundra. 

Like the name suggests, this icy layer stays solid year-round, so when it does melt, it can create big problems. The soil above the thawing permafrost can collapse, creating this wobbly, unstable surface.

7 feet above sea level: As the permafrost thaws, the soil above it can fall away. 

Along the banks of the Itkillik River in Alaska, thawing permafrost has dripped into the water, eroding the cliff side. Known as the “Stinky Bluffs,” this permafrost contains lots of frozen organic matter from dead plants and animals. As the permafrost thaws, this organic matter doesn’t just smell, it also releases carbon dioxide and methane into the atmosphere, adding to the warming effect.

446 feet above sea level: Wildfires aren’t unusual in the forests and shrub lands of Alaska, but as the climate continues to warm, they burn longer and do more damage. 

People who live off the land in the region help researchers understand where plant life isn’t growing back after fires.

100-1000 feet above sea level: Researchers set up 100-foot tall towers at strategic locations throughout Alaska to measure carbon dioxide and methane emissions from right above the forest canopy. 

This provides an up-close look at what gases are released or absorbed from the trees, or swirl in from neighboring regions. These data are combined with measurements taken from airplanes and satellites to create a clearer picture of how much carbon is entering the atmosphere.

3,369 feet above sea level: Dall sheep live in several Alaskan mountain ranges, where they’re critical to both the tourism and sports hunting economies. 

Credit: National Park Service

Changes in temperature and vegetation can profoundly affect their behavior, like grazing habits, and so researchers study how changing plant life and snow cover affect the sheep.

100-30,000 feet above sea level: Carbon emissions in the air come from thawing permafrost, fossil fuel burning, decaying vegetation and wildfires burning across the Arctic-boreal regions. 

One experiment in the ABoVE campaign measures these emissions with instruments on a DC-8 plane.

About 30,000 feet about sea level: When wildfires burn through vegetation, the effects extend far beyond what we see on the ground. 

Fires release carbon stored in the plants into the atmosphere, where it affects air quality and contributes to the greenhouse effect.

438 miles: Our ABoVE campaign combines research on the ground and from planes with data collected by a fleet of Earth-observing satellites, orbiting Earth hundreds of miles above the surface. 

Data from these satellites provides information on vegetation, atmospheric particles and gasses, and how humans are impacting our planet. With all these data sets analyzed by computer programs, the result is a comprehensive picture of our warming planet.

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Curious about NASA’s next mission to the Red Planet – the Mars 2020 Perseverance rover? Here’s your chance to ask an expert!

Targeted for launch to the Red Planet in July 2020, our Mars 2020 Perseverance rover will search for signs of ancient life. Mission engineer Lauren DuCharme and astrobiologist Sarah Stewart Johnson will be taking your questions in an Answer Time session on Friday, July 17 from noon to 1pm ET here on our Tumblr! Make sure to ask your question now by visiting http://nasa.tumblr.com/ask

Lauren DuCharme is a systems engineer at NASA’s Jet Propulsion Laboratory (JPL) in Southern California, where she’s working on the launch and cruise of the Perseverance rover. Lauren got her start at JPL as an intern. Professor Sarah Stewart Johnson is an astrobiologist at Georgetown University in Washington. Her research focuses on detecting biosignatures, or traces of life, in planetary environments.

Fun Facts:

The name Perseverance was chosen from among the 28,000 essays submitted during the "Name the Rover" contest. Seventh-grader Alex Mather wrote in his winning essay, "We are a species of explorers, and we will meet many setbacks on the way to Mars. However, we can persevere. We, not as a nation but as humans, will not give up."

Perseverance will land in Jezero Crater, a 28-mile-wide (45-kilometer-wide) crater that scientists believe was once filled with water.

Perseverance carries instruments and technology that will pave the way for future human missions to the Moon and Mars. It is also carrying 23 cameras and two microphones to the Red Planet — the most ever flown in the history of deep-space exploration.

Perseverance is the first leg of a round trip to Mars. It will be the first rover to bring a sample caching system to Mars that will package promising samples for return to Earth by a future mission.

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Have You Ever Seen An Eclipse From Space? Check It Out

On June 21, 2020 an annular solar eclipse passed over parts of Asia and Africa. Eclipses happen when the Moon lines up just right between the Sun and Earth, allowing it to block out part or all of the Sun’s bright face and cast a shadow on Earth. 

On that day, the International Space Station was orbiting over Kazakhstan and into China when this picture of the solar eclipse shadowing a portion of the Asian continent was captured by an external high definition camera. In the left foreground, is the H-II Transfer Vehicle-9 from Japan.

Here is another angle as seen from the orbital lab. In the left foreground, is the Progress 74 resupply ship from Russia.

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You don't necessarily need fancy equipment to watch one of the sky's most awesome shows: a solar eclipse. With just a few simple supplies, you can make a pinhole camera that allows you to view the event safely and easily. Before you get started, remember: You should never look at the Sun directly without equipment that's specifically designed for solar viewing. Do not use standard binoculars or telescopes to watch the eclipse, as the light could severely damage your eyes. Sunglasses also do NOT count as protection when attempting to look directly at the Sun. Stay safe and still enjoy the Sun's stellar show by creating your very own pinhole camera. It's easy! 

See another pinhole camera tutorial at https://www.jpl.nasa.gov/edu/learn/project/how-to-make-a-pinhole-camera/

Watch this and other eclipse videos on our YouTube channel:  https://youtu.be/vWMf5rYDgpc?list=PL_8hVmWnP_O2oVpjXjd_5De4EalioxAUi

A pinhole camera is just one of many viewing options. Learn more at https://eclipse2017.nasa.gov/safety 

Music credit: Apple of My Eye by Frederik Wiedmann

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Clouds swirling in the coffee colored atmosphere of Jupiter, looks more like a familiar morning beverage of champions. 

This image from our Juno spacecraft was captured in North North Temperate Belt. Image Credit: Enhanced Image by Gerald Eichstädt and Sean Doran (CC BY-NC-SA)/NASA/JPL-Caltech/SwRI/MSSS

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... and we’re ‘GO’ for launch! 🚀

NASA Flight Integration Chief and past Mission Control Flight Director, Ginger Kerrick, is here answering your questions during this Tumblr Answer Time. Tune in and join the fun!

25 Years in Space for ESA & NASA’s Sun-Watching SOHO

A quarter-century ago, the Solar and Heliospheric Observatory (SOHO) launched to space. Its 25 years of data have changed the way we think about the Sun — illuminating everything from the Sun’s inner workings to the constant changes in its outermost atmosphere.

SOHO — a joint mission of the European Space Agency and NASA — carries 12 instruments to study different aspects of the Sun. One of the gamechangers was SOHO’s coronagraph, a type of instrument that uses a solid disk to block out the bright face of the Sun and reveal the relatively faint outer atmosphere, the corona. With SOHO’s coronagraph, scientists could image giant eruptions of solar material and magnetic fields, called coronal mass ejections, or CMEs. SOHO’s images revealed shape and structure of CMEs in breathtaking detail.

These solar storms can impact robotic spacecraft in their path, or — when intense and aimed at Earth — threaten astronauts on spacewalks and even disrupt power grids on the ground. SOHO is particularly useful in viewing Earth-bound storms, called halo CMEs — so called because when a CME barrels toward us on Earth, it appears circular, surrounding the Sun, much like watching a balloon inflate by looking down on it.

Before SOHO, the scientific community debated whether or not it was even possible to witness a CME coming straight toward us. Today, SOHO images are the backbone of space weather prediction models, regularly used in forecasting the impacts of space weather events traveling toward Earth.

Beyond the day-to-day monitoring of space weather, SOHO has been able to provide insight about our dynamic Sun on longer timescales as well. With 25 years under its belt, SOHO has observed a full magnetic cycle — when the Sun’s magnetic poles switch places and then flip back again, a process that takes about 22 years in total. This trove of data has led to revolutions in solar science: from revelations about the behavior of the solar core to new insight into space weather events that explode from the Sun and travel throughout the solar system.

Data from SOHO, sonified by the Stanford Experimental Physics Lab, captures the Sun’s natural vibrations and provides scientists with a concrete representation of its dynamic movements.

The legacy of SOHO’s instruments — such as the extreme ultraviolet imager, the first of its kind to fly in orbit — also paved the way for the next generation of NASA solar satellites, like the Solar Dynamics Observatory and STEREO. Even with these newer instruments now in orbit, SOHO’s data remains an invaluable part of solar science, producing nearly 200 scientific papers every year.

Relatively early in its mission, SOHO had a brush with catastrophe. During a routine calibration procedure in June 1998, the operations team lost contact with the spacecraft. With the help of a radio telescope in Arecibo, the team eventually located SOHO and brought it back online by November of that year. But luck only held out so long: Complications from the near loss emerged just weeks later, when all three gyroscopes — which help the spacecraft point in the right direction — failed. The spacecraft was no longer stabilized. Undaunted, the team’s software engineers developed a new program that would stabilize the spacecraft without the gyroscopes. SOHO resumed normal operations in February 1999, becoming the first spacecraft of its kind to function without gyroscopes.

SOHO’s coronagraph have also helped the Sun-studying mission become the greatest comet finder of all time. The mission’s data has revealed more than 4,000 comets to date, many of which were found by citizen scientists. SOHO’s online data during the early days of the mission made it possible for anyone to carefully scrutinize a image and potentially spot a comet heading toward the Sun. Amateur astronomers from across the globe joined the hunt and began sending their findings to the SOHO team. To ease the burden on their inboxes, the team created the SOHO Sungrazer Project, where citizen scientists could share their findings.

Keep up with the latest SOHO findings at nasa.gov/soho, and follow along with @NASASun on Twitter and facebook.com/NASASunScience.

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What Astronauts in Space Eat in a Day

There was a time when even NASA didn’t know if humans could eat in the microgravity environment of space. Thankfully for the future of long-term crewed missions, John Glenn proved that it was indeed possible when he ate applesauce from an aluminum tube while orbiting the Earth in 1962.

Since then, the research conducted at our Space Food Systems Laboratory at Johnson Space Center has resulted in improved taste, variety and packaging of foods intended for space travel. Current-day astronauts are now given a standard menu of over 200 approved food and drink items months before launch, allowing them to plan their daily meals far in advance.

So, with such a variety of foods to choose from, what does the typical astronaut eat in a day?  Here is an example from the International Space Station standard menu:

Sounds tasty, right?

However, these are only suggestions for astronauts, so they still have some choice over what they ultimately eat. Many astronauts, including Tim Kopra, combine different ingredients for meals.

Others plan to eat special foods for the holidays. Astronauts Scott Kelly and Kjell Lindgren did just that on Thanksgiving last year when they ate smoked turkey, candied yams, corn and potatoes au gratin.

Another key factor that influences what astronauts eat is the availability of fresh fruits and vegetables, which are delivered via resupply spacecrafts.  When these foods arrive to the space station, they must be eaten quickly before they spoil. Astronaut Tim Peake doesn’t seem to mind.

Nutrition is important to help counteract some of the effects spaceflight have on the body, such as bone and muscle loss, cardiovascular degradation, impairment of immune function, neurovestibular changes and vision changes. 

“Nutrition is vital to the mission,” Scott M. Smith, Ph.D., manager for NASA’s Nutritional Biochemistry Lab said. “Without proper nutrition for the astronauts, the mission will fail. It’s that simple.”

We work hard to help astronauts feel less homesick by providing them with food that not only reminds them of life back on Earth, but is also nutritious and healthy. 

Here are some unusual space food inventions that are no longer in use:

Gelatin-coated sandwich and cookie cubes

Compressed bacon squares

Freeze dried ice cream

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Galactic Ghouls and Stellar Screams

A quiet, starry night sky might not seem like a very eerie spectacle, but space can be a creepy place! Monsters lurk in the shadowy depths of the universe, sometimes hidden in plain sight. Many of them are invisible to our eyes, so we have to use special telescopes to see them. Read on to discover some of these strange cosmic beasts, but beware — sometimes fact is scarier than fiction.

Monster Black Holes ⚫

You know those nightmares where no matter how fast you try to run you never seem to get anywhere? Black holes are a sinister possible version of that dream — especially because they’re real! If you get too close to a black hole, there is no possibility of escape.

Just last year our Fermi Gamma-ray Space Telescope traced an otherworldly ghost particle back to one of these monster black holes, providing additional insight into the many signals we’re picking up from some of the most feared creatures in the cosmic deep.

But it gets worse. Our Hubble Space Telescope revealed that these things are hidden in the hearts of nearly every galaxy in the universe. That means supermassive black holes lurk in the shadows of the night sky in every direction you look!

A Hazy Specter 👻

This fiendish specter lives in the center of the Milky Way, haunting our galaxy’s supermassive black hole. But it’s not as scary as it looks! Our SOFIA observatory captured streamlines tracing a magnetic field that appears to be luring most of the material quietly into orbit around the black hole. In other galaxies, magnetic fields seem to be feeding material into hungry black holes — beware! Magnetic fields might be the answer to why some black holes are starving while others are feasting.

Bats in the Belfry 🦇

The universe has bats in the attic! Hubble spotted the shadow of a giant cosmic bat in the Serpens Nebula. Newborn stars like the one at the center of the bat, called HBC 672, are surrounded by disks of material, which are hard to study directly. The shadows they cast, like the bat, can clue scientists in on things like the disk’s size and density. Our solar system formed from the same type of disk of material, but we can only see the end result of planet building here — we want to learn more about the process!

Jack-o-lantern Sun 🎃

A jack-o-lantern in space?! Our Solar Dynamics Observatory watches the Sun at all times, keeping a close eye on space weather. In October 2014, the observatory captured a chilling image of the Sun with a Halloweenish face!

Skull Comet 💀

On Halloween a few years ago, an eerie-looking object known as 2015 TB145 sped across the night sky. Scientists observing it with our Infrared Telescope Facility determined that it was most likely a dead comet. It’s important to study objects like comets and asteroids because they’re dangerous if they cross Earth’s path — just ask the dinosaurs!

Halloween Treat 🍬

Trick-or-treat! Add a piece of glowing cosmic candy to your Halloween haul, courtesy of Hubble! This image shows the Saturn Nebula, formed from the outer layers ejected by a dying star, destined to be recycled into later generations of stars and planets. Our Sun will experience a similar fate in around five billion years.

Witch’s Broom Nebula 🧹

Massive stars are in for a more fiery fate, as the Witch's Broom Nebula shows. Hubble’s close-up look reveals wisps of gas — shrapnel leftover from a supernova explosion. Astronomers believe that a couple of supernovae occur each century in galaxies like our own Milky Way.

Zombie Stars 🧟

Supernovae usually herald the death of a star, but on a few occasions astronomers have found “zombie stars” left behind after unusually weak supernovae. Our Nuclear Spectroscopic Telescope Array (NuSTAR) has even spotted a mysterious glow of high-energy X-rays that could be the “howls” of dead stars as they feed on their neighbors.

Intergalactic Ghost Towns 🏚️

The universe is brimming with galaxies, but it’s also speckled with some enormous empty pockets of space, too. These giant ghost towns, called voids, may be some of the largest things in the cosmos, and since the universe is expanding, galaxies are racing even farther away from each other all the time! Be grateful for your place in space — the shadowy patches of the universe are dreadful lonely scenes.

Mysterious Invisible Force 🕵️‍♀️

Some forces are a lot creepier than floorboards creaking or a door slamming shut unexpectedly when you’re home alone. Dark energy is a mysterious antigravity pressure that our Wide Field Infrared Survey Telescope (WFIRST) is going to help us understand. All we know so far is that it’s present everywhere in the cosmos (even in the room with you as you read this) and it controls the fate of the universe, but WFIRST will study hundreds of millions of galaxies to figure out just what dark energy is up to.

Want to learn some fun ways to celebrate Halloween in (NASA) style? Check out this link!

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High (Like 240,000 Miles) Fashion: What Astronauts Wear to the Moon

We call it a spacesuit, almost as if it’s something an astronaut pulls out of the closet. It’s more accurate to think of it as an astronaut’s personal spacecraft: self-contained and functional, with a design focused on letting astronauts work safely in space. Just as we’ve been able to improve rockets, satellites and data systems over 60 years, we’ve made great improvements to spacesuits.

When the first woman and next man step foot on the Moon in 2024, they will be wearing the next generation of spacesuit, called the Exploration Extravehicular Mobility Unit, or xEMU for short. The new suit can be used under different conditions for various tasks, including walking, driving rovers or collecting samples. The design will also allow the suits to be used for spacewalks on the space station, or Gateway – our upcoming spaceship that will orbit the Moon. Future missions to Mars can build on the core suit technologies with additional upgrades for use in the Martian atmosphere and greater gravity.

60 Years of Improvements

Even before we had astronauts, pilots were using pressurized suits to fly at high speeds at altitudes where the air was too thin to breathe. Our first spacesuits – shown here worn by the first NASA astronauts in 1959 – were variations of the suit used by Navy test pilots.

The Gemini spacesuit – shown here in a photo of astronaut Ed White making the first American spacewalk in 1965  – added a line that could connect the astronaut to the spacecraft for oxygen, and which also served as a tether when they left the capsule for a spacewalk.

The Apollo astronauts had to completely separate themselves from the lunar module, so we added a portable life support unit, which the astronauts carried on their backs. The photo above shows the life support system on the suit of Apollo 11 astronaut Buzz Aldrin as he deploys lunar experiments in 1969.

Though the bulky suits weren’t exactly easy to maneuver, astronauts still managed to get their jobs done and enjoy themselves doing it.

A Great Moment in Spacesuit History: Singing on the Moon

What, you wouldn’t sing if you were on the moon?

Different Suits for Different Functions

We have used different suits for different purposes. During the Space Shuttle program, astronauts inside the shuttle wore these orange “pumpkin” suits, which were designed to be worn within the cabin. 

On spacewalks, special suits – made to be worn only outside the spacecraft – provided high mobility, more flexibility and life support as the astronauts worked in zero gravity.

During construction of the International Space Station, we should have issued a hard hat and a pair of steel-toed boots with each suit. Astronauts conducted more than 200 spacewalks as part of building the station, which took place from 1998 until 2011. Above, an astronaut at the end of the shuttle’s robotic arm is maneuvered back into the shuttle’s payload bay with a failed pump during the shuttle’s final flight in 2011.

#MissionAccomplished

Spacesuits are rarely the story themselves, but they make it possible for our astronauts to get their jobs done, even when they have to improvise. In the picture above, astronauts on a 1992 space shuttle mission are conducting a spacewalk they hadn’t originally planned on. The crew was originally supposed to use a specially designed grab bar to capture the INTELSAT VI satellite. Two attempts to use the grab bar on two-person spacewalks failed, so we improvised a plan to add a third spacewalker and have all three go outside and literally grab the satellite.

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